Binary neutron star mergers in massive scalar-tensor theory: Properties of post-merger remnants

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Hauptverfasser: Lam, Alan Tsz-Lok, Kuan, Hao-Jui, Shibata, Masaru, Van Aelst, Karim, Kiuchi, Kenta
Format: Preprint
Veröffentlicht: 2024
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author Lam, Alan Tsz-Lok
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
author_facet Lam, Alan Tsz-Lok
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
contents We investigate the properties of post-merger remnants of binary neutron star mergers in the framework of Damour-Esposito-Farese-type scalar-tensor theory of gravity with a massive scalar field by numerical relativity simulation. It is found that the threshold mass for prompt collapse is raised in the presence of the excited scalar field. Our simulation results also suggest the existence of long-lived $ϕ-$mode in hypermassive neutron stars due to the presence of the massive scalar field which enhances the quasi-radial oscillation in the remnant. We investigate the descalarization condition in hypermassive neutron stars and discover a distinctive signature in post-merger gravitational waves.
format Preprint
id arxiv_https___arxiv_org_abs_2406_05211
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Binary neutron star mergers in massive scalar-tensor theory: Properties of post-merger remnants
Lam, Alan Tsz-Lok
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
We investigate the properties of post-merger remnants of binary neutron star mergers in the framework of Damour-Esposito-Farese-type scalar-tensor theory of gravity with a massive scalar field by numerical relativity simulation. It is found that the threshold mass for prompt collapse is raised in the presence of the excited scalar field. Our simulation results also suggest the existence of long-lived $ϕ-$mode in hypermassive neutron stars due to the presence of the massive scalar field which enhances the quasi-radial oscillation in the remnant. We investigate the descalarization condition in hypermassive neutron stars and discover a distinctive signature in post-merger gravitational waves.
title Binary neutron star mergers in massive scalar-tensor theory: Properties of post-merger remnants
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2406.05211